The analysis of the e.m. component of EAS and of the deep underground muons detected in coincidence by EAS-TOP and MACRO has been performed to study the primary cosmic ray composition in the energy range 5 · 1014 − 1 · 1016eV, around the knee of the primary spectrum. New results are presented with improved statistics, mostly above the knee of the energy spectrum.

Ambrosio, M., Antolini, R., Assiro, R., Auriemma, G., Bakari, D., Baldini, A., et al. (1996). Study of the primary cosmic ray composition around 1000 TeV with EAS-TOP and MACRO. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 48, 450-452 [10.1016/0920-5632(96)00288-5,].

Study of the primary cosmic ray composition around 1000 TeV with EAS-TOP and MACRO

BUSSINO, Severino Angelo Maria;
1996-01-01

Abstract

The analysis of the e.m. component of EAS and of the deep underground muons detected in coincidence by EAS-TOP and MACRO has been performed to study the primary cosmic ray composition in the energy range 5 · 1014 − 1 · 1016eV, around the knee of the primary spectrum. New results are presented with improved statistics, mostly above the knee of the energy spectrum.
1996
Ambrosio, M., Antolini, R., Assiro, R., Auriemma, G., Bakari, D., Baldini, A., et al. (1996). Study of the primary cosmic ray composition around 1000 TeV with EAS-TOP and MACRO. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 48, 450-452 [10.1016/0920-5632(96)00288-5,].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/120524
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